Motion of a space station. I
From MaRDI portal
Publication:5637936
DOI10.1007/BF01231403zbMath0229.70029OpenAlexW2091996789MaRDI QIDQ5637936
Giorgio Eugenio Oscare Giacaglia, William H. Jefferys
Publication date: 1971
Published in: Celestial Mechanics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf01231403
Related Items (12)
The theory of canonical perturbations applied to attitude dynamics and to the Earth rotation. Osculating and nonosculating Andoyer variables ⋮ Mutual potential between two rigid bodies with arbitrary shapes and mass distributions ⋮ Mutual gravitational potential, force, and torque of a homogeneous polyhedron and an extended body: an application to binary asteroids ⋮ Accelerating binary asteroid system propagation via nested interpolation method ⋮ The Serret-Andoyer formalism in rigid-body dynamics. I. Symmetries and perturbations ⋮ The Serret-Andoyer formalism in rigid-body dynamics. II. Geometry, stabilization, and control ⋮ Mutual gravitational potential and torque of solid bodies via inertia integrals ⋮ An expansion in power series of mutual potential for gravitating bodies with finite sizes ⋮ Vector potentials for the gravitational interaction of extended bodies and laminas with analytical solutions for two disks ⋮ A finite element method for computational full two-body problem. I: The mutual potential and derivatives over bilinear tetrahedron elements ⋮ Mutual gravitational potential ofN solid bodies ⋮ The mutual potential and gravitational torques of two bodies to fourth order
Cites Work
This page was built for publication: Motion of a space station. I